论文标题
二进制系统中的高磁场中子星和磁铁
High magnetic field neutron stars and magnetars in binary systems
论文作者
论文摘要
在二元系统中具有高度磁化中子星的情况尚不确定。一方面，所有最好的磁铁似乎都是孤立的对象。另一方面，有许多主张基于对X射线二进制中中子星的自旋特性的模型依赖性分析或/和和/和和/和和/和和/和和/和和/和和/和和/和和/和和/和和/和/和/和/和/和/和/和/和和/和和/和和/和和/和和/和和/和和/和和/和和/和和/和和/和/和/和/和/和/和/和/和/和/和/and和/和/和/and和/和/和/和/和/and和/和/和/and”的主张。此外，还有一些结果表明，在近距离二进制系统中，中子星的磁性活性。大多数理论上的考虑因素甚至不利于存在，也不是关于活跃衰变的磁性尺度田地，中子恒星中的磁性尺度片段不超过$ \ sim10^6 $〜yrs。但是，存在场进化的替代场景。我对与二进制中具有较大磁场的中子恒星的存在有关的理论和观察结果进行了简要回顾，并讨论了未来研究的观点。
Situation with highly magnetized neutron stars in binary systems is not yet certain. On the one hand, all best studied magnetars seem to be isolated objects. On the other, there are many claims based on model-dependent analysis of spin properties or/and luminosity of neutron stars in X-ray binaries in favour of large fields. In addition, there are a few results suggesting a magnetar-like activity of neutron stars in close binary systems. Most of theoretical considerations do not favour even existence, not speaking about active decay, of magnetar-scale fields in neutron stars older than $\sim10^6$~yrs. However, alternative scenarios of the field evolution exist. I provide a brief review of theoretical and observational results related to the presence of neutron stars with large magnetic field in binaries and discuss perspectives of future studies.
